The Physics of Chromospheric Plasmas: Proceedings of the Coimbra Solar Physics Meeting Held at the University of Coimbra, Coimbra, Portugal, 9-13 October, 2006Petr Heinzel, Ivan Dorotovič, Robert J. Rutten Astronomical Society of the Pacific, 2007 - 653 ページ |
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... transition region in mossy and non - mossy active - region plage . We carefully align image sequences taken with the Transition Region And Coronal Explorer ( TRACE ) in the ultraviolet passbands around 1550 , 1600 , and 1700 Å and the ...
... transition region in mossy and non - mossy active - region plage . We carefully align image sequences taken with the Transition Region And Coronal Explorer ( TRACE ) in the ultraviolet passbands around 1550 , 1600 , and 1700 Å and the ...
187 ページ
... transition region , and , dependant on the wave period , are transmitted into the lower corona . It was found that for periods close to the lower atmospheric resonant cavity period , reflection from the transition region and trapping ...
... transition region , and , dependant on the wave period , are transmitted into the lower corona . It was found that for periods close to the lower atmospheric resonant cavity period , reflection from the transition region and trapping ...
191 ページ
... transition region of the solar atmosphere . ( b ) Zoom in of a snapshot of the transition region , showing the propagation of surface gravity waves along the thin transition zone . Local velocity vectors are over - plotted . the ...
... transition region of the solar atmosphere . ( b ) Zoom in of a snapshot of the transition region , showing the propagation of surface gravity waves along the thin transition zone . Local velocity vectors are over - plotted . the ...
目次
Eightieth Anniversary of Solar Physics at Coimbra | 3 |
Spectroheliographic Observations in Madrid 19121917 | 17 |
Modeling the Solar Chromosphere | 49 |
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2007 Petr Heinzel active region arcsec ASP Conf ASP Conference Series Avrett bipoles bright calculated Carlsson chromosphere cloud model Coimbra computed continuum coronal Czech Republic density Doppler Dorotovič and Robert dynamic electron beam emission energy evolution fibrils field lines Figure filament filter filtergrams flux Fontenla Hanle effect Hansteen heating height instrument intensity inversion ionization Ivan Dorotovič limb line profiles loops magnetic field Meudon mirror motion mottles non-LTE non-thermal observations Observatory obtained optical depth optical thickness panel parameters phase photosphere pixels plage plasma polarization Pontieu prominence quiet Sun radiation radiative transfer RHESSI Rutten Schmieder shows simulations slit Solanki solar activity solar atmosphere solar disk solar flares Solar Phys Solar Prominences source function spatial resolution spectral lines spectrograph spectroheliograms spectrum Stokes structure SUMER sunspot telescope temperature transition region Trujillo Bueno variations velocity vertical wavelength waves Zeeman effect